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Re: LF: RE: Todmorden receiver

To: [email protected]
Subject: Re: LF: RE: Todmorden receiver
From: [email protected]
Date: Tue, 5 Dec 2017 08:45:35 -0330 (NST)
In-reply-to: <[email protected]>
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Thank-you for the update, Paul.  It't amazing that 10 uW can be detected
over there -  almost like spooky action at a distance, with only
a few hundred billion photons per second.

The carrier is phase stabilised by Spec Lab so the tuning coil can be
peaked without glitching the phase and the current is also periodically
adjusted to keep it about 0.25A.  Is it possible to see diurnal changes
in the phase?

The TX will be on for the weekend for Stefan's VLF party unless the
wx gets in the way.

73
Joe VO1NA

On Tue, 5 Dec 2017, Paul Nicholson wrote:


New H-field rx is coming along well.  Design changes are
completed - it has a lower system noise, wider bandwidth,
significantly lower common mode response, and a much better
line driver.  Like the new E-field rx, it also has a built-in
calibration port.

Currently testing the design changes on breadboard and it
performs just as per the Spice model, except for a higher than
expected system noise.   Should be just below 0.1fT in 1Hz
but I'm measuring 0.46 fT.   Maybe this specimen of LT1028
is a bit noisier than others?  It's my last one but I've
got more arriving hopefully today.   I'll pick the best two.
Even with this mysterious extra system noise, it's still 20dB
below the natural noise floor after sferic blanking.

Apart from that it is working perfectly, just as per design
and looks very good at 137 kHz too.

Hopefully will be able to start the cutting and drilling and
filing and soldering this week.  That's my least favourite part
of the job.

What I won't discover until it's finished and installed, is
whether it actually cures the excess noise at 8kHz and 5kHz
that we've seen lately.  I haven't been able to identify the
cause of the relatively (compared to E-field) poor S/N on the
existing rx.  Hopefully it is a low level of intermod in the
line driver.  If so the new rx will not suffer that problem
and we'll see another step improvement in the 8270 spectrogram.

--
Paul Nicholson
--



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